J/ApJ/810/166 RESOLVE survey photometry catalog (Eckert+, 2015)
RESOLVE survey photometry and volume-limited calibration of
the photometric gas fractions technique.
Eckert K.D., Kannappan S.J., Stark D.V., Moffett A.J., Norris M.A.,
Snyder E.M., Hoversten E.A.
<Astrophys. J., 810, 166 (2015)>
=2015ApJ...810..166E 2015ApJ...810..166E (SIMBAD/NED BibCode)
ADC_Keywords: Galaxy catalogs ; Photometry, ugriz ; Photometry, infrared ;
Photometry, ultraviolet ; Redshifts
Keywords: galaxies: ISM; galaxies: photometry; surveys
Abstract:
We present custom-processed ultraviolet, optical, and near-infrared
photometry for the REsolved Spectroscopy of a Local VolumE (RESOLVE)
survey, a volume-limited census of stellar, gas, and dynamical mass
within two subvolumes of the nearby universe (RESOLVE-A and
RESOLVE-B). RESOLVE is complete down to baryonic mass
∼109.1-9.3M☉, probing the upper end of the dwarf galaxy
regime. In contrast to standard pipeline photometry (e.g., SDSS), our
photometry uses optimal background subtraction, avoids suppressing
color gradients, and employs multiple flux extrapolation routines to
estimate systematic errors. With these improvements, we measure
brighter magnitudes, larger radii, bluer colors, and a real increase
in scatter around the red sequence. Combining stellar mass estimates
based on our optimized photometry with the nearly complete HI mass
census for RESOLVE-A, we create new z=0 volume-limited calibrations of
the photometric gas fractions (PGF) technique, which predicts
gas-to-stellar mass ratios (G/S) from galaxy colors and optional
additional parameters. We analyze G/S-color residuals versus potential
third parameters, finding that axial ratio is the best independent and
physically meaningful third parameter. We define a "modified color"
from planar fits to G/S as a function of both color and axial ratio.
In the complete galaxy population, upper limits on G/S bias linear and
planar fits. We therefore model the entire PGF probability density
field, enabling iterative statistical modeling of upper limits and
prediction of full G/S probability distributions for individual
galaxies. These distributions have two-component structure in the red
color regime. Finally, we use the RESOLVE-B 21cm census to test
several PGF calibrations, finding that most systematically under- or
overestimate gas masses, but the full probability density method
performs well.
Description:
The RESOLVE survey (Kannappan & Wei 2008AIPC.1035..163K 2008AIPC.1035..163K; Kannappan+
2015, in preparation) is located within the SDSS footprint and makes
use of the SDSS redshift survey to build up survey membership with
completeness down to Mr,petro=-17.23, the absolute r-band magnitude
corresponding to the SDSS survey limit of mr,petro=17.77 at the
outer RESOLVE cz limit, 7000km/s. We also include additional redshifts
from various archival sources.
The RESOLVE-A data (the A-semester) set shown in Figure 1(a) occupies
a volume of ∼38400Mpc3 defined by: 131.25°<RAJ2000<236.25°,
0°<DEJ2000<5°, and 4500km/s<cz<7000km/s.
The RESOLVE-B data set is located in the SDSS Stripe 82 equatorial
region, and it occupies a smaller volume of ∼13700Mpc3 defined by:
22h<RAJ2000<3h, -1.25°<DEC<1.25°, and 4500km/s<cz<7000km/s.
File Summary:
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FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
table1.dat 397 2286 REsolved Spectroscopy of a Local VolumE (RESOLVE)
custom photometry catalog - from erratum published
in 2017, ApJ, 847, 83
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See also:
II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)
II/312 : GALEX-DR5 (GR5) sources from AIS and MIS (Bianchi+ 2011)
VII/259 : 6dF galaxy survey final redshift release (Jones+, 2009)
VIII/77 : HI spectral properties of galaxies (Springob+, 2005)
VII/237 : HYPERLEDA. I. Catalog of galaxies (Paturel+, 2003)
VII/250 : The 2dF Galaxy Redshift Survey (2dFGRS) (2dFGRS Team, 1998-2003)
J/MNRAS/436/34 : GALEX Arecibo SDSS survey. Final release (Catinella+, 2013)
J/ApJ/777/42 : Kinematic and HI data for the NFGS (Kannappan+, 2013)
J/ApJ/769/82 : H2 masses in a broad sample of galaxies (Stark+, 2013)
J/MNRAS/425/2741 : Parameters of Spiral galaxies from SDSS 7 (Hall+, 2012)
J/AJ/142/170 : ALFALFA survey: α.40 HI source catalog (Haynes+, 2011)
J/ApJS/196/11 : Bulge+disk decompositions of SDSS galaxies (Simard+, 2011)
J/AJ/141/205 : UVOT imaging of M81 and Holmberg IX (Hoversten+, 2011)
J/MNRAS/413/971 : Galaxy And Mass Assembly (GAMA) DR1 (Driver+, 2011)
J/MNRAS/403/683 : GALEX Arecibo SDSS survey (GASS) (Catinella+, 2010)
J/ApJ/708/841 : Star formation in E/S0 galaxies (Wei+, 2010)
J/ApJ/703/1569 : Radial distribution in SINGS gal. I. (Munoz-Mateos+, 2009)
J/MNRAS/394/1857 : H2/HI ratio in galaxies (Obreschkow+, 2009)
J/ApJS/173/538 : XUV-Disk galaxies in the Local Universe (Thilker+, 2007)
J/ApJS/167/1 : Galaxy groups and clusters from SDSS (Berlind+, 2006)
J/A+A/428/823 : HI catalog of low surface brightness gal. (O'Neil+, 2004)
J/ApJS/126/271 : Surface photometry of nearby field galaxies (Jansen+ 2000)
J/PASP/111/438 : Updated Zwicky catalog (UZC) (Falco+, 1999)
J/A+A/313/377 : Near-IR photometry of 86 galaxies. IV. (de Jong 1996)
http://www.sdss3.org/ : SDSS-III home page
Byte-by-byte Description of file: table1.dat
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Bytes Format Units Label Explanations
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1- 6 A6 --- ID RESOLVE galaxy identifier (r{f/s}NNNN)
8- 15 F8.4 deg RAdeg Right Ascension in decimal degrees (1)
17- 23 F7.4 deg DEdeg Declination in decimal degrees (1)
25- 31 F7.2 km/s cz0 [4253/7284] Local group corrected
velocity of galaxy
33- 39 F7.2 km/s cz [4178/7362] Adopted galaxy velocity for
survey membership
41- 47 F7.3 mag rMag [-23.6/-13.5] Absolute SDSS r-band
magnitude (2)
49- 55 F7.3 mag umag [13.3/27.1]? Apparent SDSS u-band
magnitude (3)
57- 63 F7.3 mag e_umag [0.02/7]? Error in umag
65- 70 F6.3 mag gmag Apparent SDSS g-band magnitude (3)
72- 78 F7.3 mag e_gmag ? Error in gmag
80- 85 F6.3 mag rmag Apparent SDSS r-band magnitude (3)
87- 91 F5.3 mag e_rmag Error in rmag
93- 98 F6.3 mag imag [10.6/20.6] Apparent SDSS i-band
magnitude (3)
100-104 F5.3 mag e_imag [0.02/3] Error in imag
106-112 F7.3 mag zmag [10.2/22.4]? Apparent SDSS z-band
magnitude (3)
114-120 F7.3 mag e_zmag [0.02/10]? Error in zmag
122-128 F7.3 mag NUVmag [14.7/25]? Apparent GALEX NUV-band
magnitude (3)
130-136 F7.3 mag e_NUVmag [0.01/7]? Error in NUVmag
138-144 F7.3 mag uvm2mag [17.5/21.7]? Apparent Swift uvm2-band
magnitude (3)
146-152 F7.3 mag e_uvm2mag [0.01/2]? Error in uvotm2mag
154-160 F7.3 mag 2Jmag [9.6/16]? Apparent 2MASS J-band
magnitude (3)
162-168 F7.3 mag e_2Jmag [0.01/5]? Error in 2Jmag
170-176 F7.3 mag 2Hmag ? Apparent 2MASS H-band magnitude (3)
178-184 F7.3 mag e_2Hmag ? Error in 2Hmag
186-192 F7.3 mag 2Kmag [8.7/15]? Apparent 2MASS K-band
magnitude (3)
194-200 F7.3 mag e_2Kmag [0.01/4]? Error in 2Kmag
202-208 F7.3 mag UYmag [10.4/20.1]? Apparent UKIDSS Y-band
magnitude (3)
210-216 F7.3 mag e_UYmag [0.005/13]? Error in UYmag
218-224 F7.3 mag UHmag [3.8/18]? Apparent UKIDSS H-band
magnitude (3)
226-232 F7.3 mag e_UHmag [0.004/10]? Error in UHmag
234-240 F7.3 mag UKmag [8.8/17.5]? Apparent UKIDSS K-band
magnitude (3)
242-248 F7.3 mag e_UKmag [0.004/13]? Error in UKmag
250-253 F4.2 --- b/a [0.1/1] The axial ratio
255-259 F5.2 arcsec R50 [1/52] The half-light radius in r band
261-266 F6.2 arcsec R90 [2/191] The 90%-light radius in r band
268-274 F7.4 mag g(g-r) [-0.7/1.3] The (g-r) color gradient
276-280 F5.3 mag modu-r [0.6/3.2] SED modeled (u-r) color (4)
282-286 F5.3 mag modu-i [0.6/3.7] SED modeled (u-i) color (4)
288-292 F5.3 mag modu-j [1.5/5.5] SED modeled (u-J) color (4)
294-298 F5.3 mag modu-k [2.2/6.5] SED modeled (u-K) color (4)
300-304 F5.3 mag modg-r [0.02/1.1] SED modeled (g-r) color (4)
306-310 F5.3 mag modg-i [0.05/1.6] SED modeled (g-i) color (4)
312-316 F5.3 mag modg-j [0.9/3.4] SED modeled (g-J) color (4)
318-322 F5.3 mag modg-k [1.6/4.4] SED modeled (g-K) color (4)
324-328 F5.2 [Msun] logM* [6.7/11.7] Log stellar mass
330-334 F5.3 mag extu [0.07/1] Foreground extinction in u band
336-340 F5.3 mag extg [0.05/0.8] Foreground extinction in g band
342-346 F5.3 mag extr [0.03/0.6] Foreground extinction in r band
348-352 F5.3 mag exti [0.03/0.4] Foreground extinction in i band
354-358 F5.3 mag extz [0.02/0.3] Foreground extinction in z band
360-365 F6.3 mag extnuv [1.3/17.6] Foreground extinction in
nuv band
367-371 F5.3 mag extuvm2 [0.1/2] Foreground extinction in uvm2 band
373-377 F5.3 mag exty [0.01/0.3] Foreground extinction in Y band
379-383 F5.3 mag extj [0.01/0.2] Foreground extinction in J band
385-389 F5.3 mag exth [0.008/0.2] Foreground extinction in H band
391-395 F5.3 mag extk [0.005/0.07] Foreground extinction
in K band
397 I1 --- Set [0/1]? Sample flag (5)
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Note (1): Photometric center of galaxy (J2000).
Note (2): Foreground extinction included.
Note (3): All magnitudes are newly measured from the raw images. Apparent
magnitudes are provided without foreground extinction corrections.
Note (4): Model colors are products of the SED fitting routine from K13
(Kannappan+, 2013, J/ApJ/777/42), described in Section 3.2 and have
foreground extinction corrections and k-corrections implicitly
included.
Note (5): Flag as follows:
1 = galaxy is in the calibration or testing sample.
0 = galaxy is not in the calibration or testing sample.
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History:
From electronic version of the journal
19-Jan-2016: Insert into VizieR
09-Oct-2017: Table 1 updated according to erratum 2017, ApJ, 847, 83
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 18-Dec-2015